1302.4363 (M. Galametz et al.)

Calibration of the total infrared luminosity of nearby galaxies from Spitzer and Herschel bands    [PDF]

M. Galametz, R. C. Kennicutt, D. Calzetti, G. Aniano, B. T. Draine, M. Boquien, B. Brandl, K. V. Croxall, D. A. Dale, C. W. Engelbracht, K. D. Gordon, B. Groves, C. -N. Hao, G. Helou, J. L. Hinz, L. K. Hunt, B. D. Johnson, Y. Li, E. Murphy, H. Roussel, K. Sandstrom, R. A. Skibba, F. S. Tabatabaei

We present new empirical calibrations to estimate resolved and integrated total infrared luminosities from Spitzer and Herschel bands used as monochromatic or combined tracers. We base our calibrations on resolved elements of nearby galaxies (3 to 30 Mpc) observed with Herschel. We perform a resolved SED modelling of these objects using the Draine and Li (2007) dust models and investigate the influence of the addition of SPIRE measurements in the estimation of LTIR. We find that using data up to 250 um leads to local LTIR values consistent with those obtained with a complete coverage (up to 500 um) within 10 per cent for most of our resolved elements. We then study the distribution of energy in the resolved SEDs of our galaxies. The bulk of energy (30-50 per cent) is contained in the (70-160 um) band. The (24-70 um) fraction decreases with increasing metallicity. The (160-1100 um) submillimeter band can account for up to 25 per cent of the LTIR in metal-rich galaxies. We investigate the correlation between TIR surface brightnesses/luminosities and monochromatic Spitzer and Herschel surface brightnesses/luminosities. The three PACS bands can be used as reliable monochromatic estimators of the LTIR, the 100 um band being the most reliable monochromatic tracer. There is also a strong correlation between the SPIRE 250um and LTIR, although with more scatter than for the PACS relations. We also study the ability of our monochromatic relations to reproduce integrated LTIR of nearby galaxies as well as LTIR of z=1-3 sources. Finally, we provide calibration coefficients that can be used to derive TIR surface brightnesses/luminosities from a combination of Spitzer and Herschel surface brightnesses/fluxes and analyse the associated uncertainties.

View original: http://arxiv.org/abs/1302.4363